Celestial hemisphere:  Northern  ·  Constellation: Cepheus (Cep)  ·  Contains:  HD206136  ·  HD206897  ·  IC 5134  ·  LBN 497  ·  LDN 1181  ·  LDN 1183  ·  NGC 7129  ·  NGC 7133  ·  NGC 7142  ·  VdB146
Getting plate-solving status, please wait...
NGC 7129, NGC 7142 and a lot of bright stars, Massimo Di Fusco
NGC 7129, NGC 7142 and a lot of bright stars, Massimo Di Fusco

NGC 7129, NGC 7142 and a lot of bright stars

Getting plate-solving status, please wait...
NGC 7129, NGC 7142 and a lot of bright stars, Massimo Di Fusco
NGC 7129, NGC 7142 and a lot of bright stars, Massimo Di Fusco

NGC 7129, NGC 7142 and a lot of bright stars

Equipment

Loading...

Acquisition details

Loading...

Description

Even though it is the most difficult condition for me from my city sky, I just can't give up the beauty that can be achieved in broadband. 
In this image I wanted to bring into the same frame the beautiful reflection nebula NGC 7129 at the top center, the open cluster NGC 7142 at the bottom left and a group of bright stars at the bottom right. We are, of course, in the constellation Cepheus.

NGC 7129 is a star-forming region that has many interesting features. Astronomers estimate that many of the bright stars it contains are less than 1 million years old. These "baby" stars are very energetic and emit abundant amounts of radiation that excite the gas clouds that surround them. Furthermore, the very red structures that can be seen indicate regions where new stars, that are not yet visible, are forming. These regions are often outflows of gas called Herbig Haro (HH) objects (the crescent-shaped object near the lower right of the nebula is, for example, HH103; see revision B). 
Furthermore, energetic regions like this can often produce molecular masers. A maser (like a laser in visible wavelengths) is a coherent light signal in microwave wavelengths. In this case, molecules in these gas regions are excited by high-energy photons and re-emit microwaves back towards us preferentially. The fascinating thing is that the molecules in question are quite important to us: they are water molecules!

NGC 7142 is an open cluster about 6200 light years away from us. Its proximity to the reflection nebula NGC 7129 suggests that the cluster may be obscured by an interstellar cloud. And in fact, many studies have shown that this is indeed the case. This cluster is believed to be close in age to the old open clusters M67 and NGC 188 and this makes it one of the oldest open clusters currently known.

Comments